8. Mass spectra and IR Mass spectrometry Measuring the Mr of an organic molecule Spectra for C4H10 Mass spectrum for butane If a molecule is put through a mass spectrometer it will often break up and give a series of peaks caused by the fragments. The peak with the largest m/z, however, will be due to the complete molecule and will be equal to the Mr of the molecule. This peak is called the parent ion or molecular ion 43 Molecular ion C4H10+ 29 58 Fragmentation Molecular ion formed: When organic molecules are passed through a mass spectrometer, it detects both the whole molecule and fragments of the molecule. M → [M]+. + e– The molecule loses an electron and becomes both an ion and a free radical Several peaks in the mass spectrum occur due to fragmentation. The Molecular ion fragments due to covalent bonds breaking: [M]+. → X+ + Y. This process produces an ion and a free radical. The ion is responsible for the peak Relatively stable ions such as carbocations R+ such as CH3CH2+ and acylium ions [R-C=O]+ are common. The more stable the ion, the greater the peak intensity. The peak with the highest mass/charge ratio will be normally due to the original molecule that hasn’t fragmented (called the molecular ion) . As the charge of the ion is +1 the mass/ charge ratio is equal to Mr. Equation for formation molecular ion Mass spectrum for propanal 29 CH3CH2CHO → [CH3CH2CHO]+. + e– m/z 58 [CHO]+ Equations for formation of fragment ions from molecular ions 58 [CH3CH2CHO]+. Mass spectrum for propanone The high peak at 43 due to stability of acyl group 43 [CH3CO]+ [CH3COCH3]+. [CH3CH2CHO]+. → [CHO]+ + .CH2CH3 [CH3CH2CHO]+. → [CH3CH2]+ + .CHO m/z 29 m/z 29 Equation for formation molecular ion CH3COCH3 → [CH3COCH3]+. + e– m/z 58 Equations for formation of fragment ions from molecular ions [CH3COCH3]+. → [CH3CO]+ + . CH3 m/z 43 58 15 It is not possible for propanone to fragment to give a peak at 29 so the fragmentation patterns can distinguish between the structural isomers of propanone and propanal N Goalby chemrevise.org 1 Infrared spectroscopy Complicated spectra can be obtained than provide information about the types of bonds present in a molecule Certain bonds in a molecule absorb infra-red radiation at characteristic frequencies causing the covalent bonds to vibrate ABOVE 1500 cm-1 – “Functional group identification” BELOW 1500 cm-1 – “Fingerprinting” Complicated and contains many signals – picking out functional group signals difficult. This part of the spectrum is unique for every compound, and so can be used as a "fingerprint". e.g. C=O 1640 – 1750 cm-1 A computer will compare the IR spectra against a database of known pure compounds to identify the compound O-H (acid) 2500- 3300 cm-1 Use an IR absorption table provided in exam to deduce presence or absence of particular bonds or functional groups Bond Wavenumber C-O 1000-1300 C=O 1640-1750 C-H 2850 -3100 O-H Carboxylic acids 2500-3300 Very broad N-H 3200-3500 O-H Acohols, phenols 3200- 3550 broad Use spectra to identify particular functional groups e.g. an alcohol from an absorption peak of the O–H bond, or C=O stretching absorption in aldehydes and ketones Spectra for butanal O H3C CH2 CH2 C 2000 1500 C=O Absorption or trough in between 1640-1750 cm-1 range indicates presence of C=O bond N Goalby chemrevise.org 2 H Always quote the wave number range from the data sheet Spectra for ethanoic acid O-H absorptions tend to be broad O Absorption or trough in between 2500-3300 cm-1 range indicates presence of O-H bond in an acid H3C C OH C=O Absorption or trough in between 16401750 cm-1 range indicates presence of C=O bond Molecules which change their polarity as they vibrate can absorb infrared radiation. E.g. C-H, C=O, O-H Molecules such as H2, O2 and N2 cannot change their polarity as they vibrate so can absorb infrared radiation and don’t register on an infra red spectrum The absorption of infra-red radiation by bonds in this type of spectroscopy is the same absorption that bonds in CO2, methane and water vapour in the atmosphere do that cause them to be greenhouse gases. H2O, CO2, CH4 and NO molecules absorb IR radiation and are greenhouse gases, whilst O2 and N2 are not. N Goalby chemrevise.org 3
© Copyright 2026 Paperzz